The first two transient supersoft X-ray sources in M 31 globular clusters and the connection to classical novae

Astronomy and Astrophysics

Volumn 500, Issue 2, 2009, Pages 769-779

  Henze, M ^a   Pietsch, W ^a   Haberl, F ^a   Sala, G ^a,b   Quimby, R ^c,l   Hernanz, M ^d   Della Valle, M ^e,f,g   Milne, P ^h   Williams, G G ^h   Burwitz, V ^a   Greiner, J ^a   Stiele, H ^a   Hartmann, D H ⁱ   Kong, A K H ^j   Hornoch, K ^k  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b UNIVERSITAT POLITÈCNICA DE CATALUNYA   (Spain)

^c UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^d INSTITUT DE CIÈNCIES DE L ESPAI CSIC IEEC   (Spain)

^e EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^f INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^g ICRANET   (Italy)

^h UNIVERSITY OF ARIZONA   (United States)

ⁱ CLEMSON UNIVERSITY   (United States)

^j NATIONAL TSING HUA UNIVERSITY   (Taiwan)

^k ASTRONOMICAL INSTITUTE   (Czech Republic)

^l CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

Globular clusters, individual. Bol 194 ; Novae; Stars, individual: Nova m31n 2007; 06b globular clusters, individual, bol 111; Cataclysmic variables; Galaxies, individual, m 31; X rays, galaxies

Indexed keywords

- GLOBULAR CLUSTERS, INDIVIDUAL. BOL 194 -; - NOVAE; - STARS, INDIVIDUAL: NOVA M31N 2007; -06B GLOBULAR CLUSTERS, INDIVIDUAL, BOL 111; CATACLYSMIC VARIABLES; X-RAYS, GALAXIES;

ELECTRON SOURCES; GALAXIES; STARS; X RAY APPARATUS;

X RAYS;

EID: 67649526102     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811122     Document Type: Article

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